Comparison between different grid models and the goodness of fit for the MnS (top row), MgSiO₃ (middle row), and Fe (bottom row) clouds calculated at the planetary radius set to 2.313 R_⊕. For each species, the left panel shows our observations with uncertainties compared against some selected lowest reduced chi-squared (${\chi }_{\nu }^2$) models, with the corresponding ${\chi }_{\nu }^2$ values in the bottom legend. The parameter values for clear, no-cloud models are given in the left legend, and for cloudy models, they are given in the right legend. The flat model is drawn as a dotted line at a transit depth of 418 ppm. The tables in the middle and right panels display the models’ ${\chi }_{\nu }^2$ values on a grid of cloud droplet radius r_g, droplet volume mixing ratio q*, and metallicity [M/H]. The table titles list fixed parameters. The color bar extent is set between 1 and 2 to highlight only the models that best fit the data.